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Woo, K. Mori, K. Pfrang, K. Ragan, L. Saha, M. Abdelmaguid, M. Capasso, M. J. Lang, M. Kertzman, M. Pohl, N. Korzoun, N. Park, O. Hervet, P. Batista, P. Kaaret, P. Moriarty, P. T. Reynolds, Q. Feng, R. A. Ong, R. Mukherjee, S. Kumar, S. O'Brien, S. P. Reynolds, S. R. Patel, S. Safi-Harb, T. B. Humensky, T. K. Kleiner, VERITAS Collaboration: P. Bangale, W. Benbow, W. F Hanlon, W. Jin","submitted_at":"2023-10-06T18:10:14Z","abstract_excerpt":"G106.3$+$2.7, commonly considered a composite supernova remnant (SNR), is characterized by a boomerang-shaped pulsar wind nebula (PWN) and two distinct (\"head\" & \"tail\") regions in the radio band. A discovery of very-high-energy (VHE) gamma-ray emission ($E_\\gamma > 100$ GeV) followed by the recent detection of ultra-high-energy (UHE) gamma-ray emission ($E_\\gamma > 100$ TeV) from the tail region suggests that G106.3$+$2.7 is a PeVatron candidate. 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Falcone, A. J. Chromey, A. Weinstein, C. E McGrath, C. J. Hailey, C. L. Mooney, D. A. Williams, D. Hanna, D. Kieda, D. Tak, E. Pueschel, E. Roache, F. Krennrich, G. Gallagher, G. H. Sembroski, G. Maier, G. M Foote, H. An, I. Pope, I. Sadeh, J. D. Gelfand, J. H. Buckley, J. Holder, J. L. Christiansen, J. P. Finley, J. Quinn, J. V. Tucci, J. Woo, K. Mori, K. Pfrang, K. Ragan, L. Saha, M. Abdelmaguid, M. Capasso, M. J. Lang, M. Kertzman, M. Pohl, N. Korzoun, N. Park, O. Hervet, P. Batista, P. Kaaret, P. Moriarty, P. T. Reynolds, Q. Feng, R. A. Ong, R. Mukherjee, S. Kumar, S. O'Brien, S. P. Reynolds, S. R. Patel, S. Safi-Harb, T. B. Humensky, T. K. Kleiner, VERITAS Collaboration: P. Bangale, W. Benbow, W. F Hanlon, W. Jin","submitted_at":"2023-10-06T18:10:14Z","abstract_excerpt":"G106.3$+$2.7, commonly considered a composite supernova remnant (SNR), is characterized by a boomerang-shaped pulsar wind nebula (PWN) and two distinct (\"head\" & \"tail\") regions in the radio band. 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